Aug_16_1999_L25.txt Shift L25 Start at 1999:228:10:00 GMT = 1999 Aug 16 6:00am EDT End 1999 Aug 16 2:00pm EDT See http://asc.harvard.edu/acis/SOT_reports/sot-shift.html, or /proj/ascwww/AXAF/extra/science/htdocs/acis/SOT_reports/Aug_16_1999_L25.txt. SOT Lead Ed Kellogg SOT SC/ACA Rob Cameron FOT-SI HRC-SI ACIS-SI (Times will be given in GMT on day 228. not precise.) EVENTS PLAN DONE OBSID -------------- ---- ---- ----- Start shift (06am EDT 16 Aug 1999) 1000 1000 1056 Goldstone LOS 1109 1112 Madrid AOS 1720 1645 1056 New OBSID, maneuver, got 2 of 3 acq, 3 of 5 guide stars 1656 1057 New OBSID, maneuver, got 3 acq, 4 of 5 guide stars 1742 1058 End shift (2pm EDT 12 Aug) day 228 1800 NOTES/ISSUES/PROBLEMS --------------------- At H-to-L shift change, 226:1000, Chandra 2 hrs before apogee ACA tracking, one star box empty HRC EPHIN nominal ACIS Vacuum 4.5e-6 torr COM Goldstone The shift started quietly. We were in the radiation zone, and went LOS after 1 hr. We did not see real time data until ~6 hrs later. Issues being worked: * The SOT lead needs a document that gives the correct and current contents of the daily load in a readable form. We are discussing implementation with Mission Planning. * The M shift needs to make sure that CAP 284 is executed at ~2240 to disable dither for the ACA Field Distortion Coefficients measurement. * Ian Evans is reporting a "poor" aspect solution. We need to investigate that. * Because of stars not acquired in recent pointings, Rob Cameron will be analyzing the data to see if any trend emerges for the disparity between stellar receiver magnitudes in the OFLS catalog and those observed in ACA, vs. color, time, etc. It appears that the receiver magnitudes are ~1 mag fainter than the catalog magnitudes. The fidlites do not appear to be changing with time, so that probably obviates camera icing as the cause. * We need to make a permanent change in the algorithm for generating the DOT so that there will be a 3 min delay between ACIS stop science (AA00000000) and commanding the next OBSID, to allow ACIS to send down data that are transmitted after AA00000000 but belong with the previous obsid. This was communicated to CXC MP, Pat Slane. The maneuver at 1656 got 2 of 3 acquisition stars, and 3 of 5 guide stars, a bit worse than the previous maneuvers. We continue with another Crude Optical Axis Determination ACIS observation, at y_offset = 2.8', z_offset = 2.8.'